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Normal Distribution Explorer


Modify Parameters and See Results

Bell curve - the most important continuous distribution

Parameters

Mean (μ)
0.00

Center of the distribution (also median and mode)

Standard Deviation (σ)
1.00

Measure of spread around the mean

Variance (σ²)
1.00

Square of the standard deviation

Statistics

Expected Value
0.0000
Variance
1.0000
Std Deviation
1.0000
Mode
0.0000

Probability Calculator

Key Properties

Real-World Applications

  • Heights and weights of populations
  • Measurement errors in scientific experiments
  • Test scores and IQ measurements
  • Blood pressure in healthy adults
  • Manufacturing tolerances and product dimensions
  • Returns on financial investments (short-term)







Adjusting Mean and Standard Deviation

Use the μ (mu) slider to shift the distribution's center along the x-axis. Values range from -10 to 10, moving the bell curve left or right without changing its shape.

Adjust σ (sigma) slider to control spread. Smaller σ creates a tall, narrow curve with values concentrated near μ. Larger σ produces a short, wide curve with more variability.

Watch how changing these parameters affects the visualization. The curve always remains symmetric around μ, with the same bell shape regardless of parameters - only location and scale change.

Reading the PDF Curve

The PDF (Probability Density Function) displays the characteristic bell-shaped curve. The peak occurs at x = μ, representing the distribution's mean, median, and mode - all equal due to symmetry.

The curve extends from -∞ to +∞ theoretically, but the calculator shows the practical range μ ± 4σ where 99.99% of probability mass resides. Areas under the curve represent probabilities.

Inflection points (where curvature changes) occur at μ ± σ. Between these points, the curve is steepest, containing about 68% of the total probability. This geometric feature helps visualize the 68-95-99.7 rule.

Understanding the CDF Display

The CDF (Cumulative Distribution Function) shows the characteristic S-curve rising from 0 to 1. At any point x, the height gives P(X ≤ x), the probability of values at or below x.

The CDF's steepest region occurs around μ where the PDF peaks. At μ itself, CDF equals 0.5 - exactly half the probability lies below the mean due to symmetry.

The CDF approaches but never quite reaches 0 or 1 at the display's edges. At μ ± 3σ, CDF values are approximately 0.0013 and 0.9987, leaving only 0.27% probability in the extreme tails combined.

Using the Probability Calculators

Enter value x in the P(X ≤ x) calculator to find the area under the curve to the left of x. This uses the error function erf(z) where z = (x - μ)/σ is the standardized Z-score.

P(X ≥ x) gives the right-tail probability, computed as 1 - P(X ≤ x). This answers questions like "What fraction of values exceed x?"

For range probabilities P(a ≤ X ≤ b), the calculator computes CDF(b) - CDF(a), giving the area under the curve between a and b. This is the fundamental probability for any continuous interval.

Working with Z-Scores

Every normal distribution calculation uses standardization: Z = (X - μ)/σ transforms values to standard normal (μ = 0, σ = 1). The calculator performs this conversion automatically.

Z-scores measure distance from the mean in standard deviation units. Z = 2 means "2 standard deviations above the mean." Z = -1.5 means "1.5 standard deviations below."

The standard normal table (Z-table) provides CDF values for Z-scores. For any normal distribution, standardize first, then look up the Z-score. This is why one table suffices for all normal distributions.

The Empirical Rule (68-95-99.7)

The 68% rule: About 68% of values fall within μ ± σ. For μ = 100, σ = 15, expect 68% of values in [85, 115].

The 95% rule: About 95% fall within μ ± 2σ. Using the same parameters, 95% lie in [70, 130]. Only 5% of values fall more than 2 standard deviations from the mean.

The 99.7% rule: About 99.7% fall within μ ± 3σ, or [55, 145]. Values beyond ±3σ are rare, occurring less than 0.3% of the time. This rule underpins control charts and outlier detection.

What is the Normal Distribution?

The normal (Gaussian) distribution is the most important continuous probability distribution, modeling natural phenomena that result from many small, independent factors. Its bell shape appears throughout nature, science, and statistics.

Two parameters completely define it: μ (mean) determines location, σ (standard deviation) determines spread. The distribution is symmetric around μ, with probability decreasing exponentially as distance from μ increases.

The normal distribution is fundamental because of the Central Limit Theorem: sums and averages of independent random variables tend toward normality regardless of the original distribution. For comprehensive theory, see normal distribution theory page.

Central Limit Theorem Connection

The Central Limit Theorem explains why normal distributions appear so frequently. When you sum or average many independent random variables, the result approaches a normal distribution even if the original variables aren't normal.

This applies to measurement errors (sum of many small perturbations), test scores (sum of knowledge across many topics), and manufacturing tolerances (sum of variations in multiple processes).

The theorem works surprisingly quickly - often just 30 observations suffice for reasonable normality. This makes the normal distribution applicable even when underlying processes aren't purely Gaussian.

Distribution Properties and Statistics

Mean, median, and mode all equal μ due to perfect symmetry. There's no skewness - the distribution is perfectly balanced around its center.

Variance equals σ², the square of the standard deviation. Standard deviation σ is the natural scale parameter, representing typical deviation from the mean.

The distribution has zero skewness (symmetric) and kurtosis of 3 (defining "normal" tail behavior). Distributions with kurtosis > 3 have heavier tails; kurtosis < 3 have lighter tails than normal.

Related Distributions and Calculators

The standard normal distribution (Z-distribution) has μ = 0 and σ = 1, serving as the reference for all normal calculations. Any normal distribution can be standardized using Z = (X - μ)/σ.

The t-distribution approximates normal for large sample sizes but has heavier tails, accounting for additional uncertainty when estimating σ from data. Use t for small samples (n < 30).

Related Tools:

Z-Score Calculator - Standardization and percentiles

T-Distribution Calculator - Small sample inference

Chi-Square Distribution - Related to normal's squared values

Hypothesis Testing Tools - Applications of normal distribution